U 428
11:30 to 12:30
-39° to -50°
Cen, Cru
Feb-Jun

FEATURED OBJECTS: NGC 3918, NGC 3960 (Ben 48), Stock 15, NGC 4230, NGC 4337, Harvard 5, NGC 4439, Ruprecht 165, Hogg 14.

NGC 3918
ESO170-PN013, PK294+04.01
RA 11:50:16
Dec -57° 04.5'
Planetary nebula

This planetary nebula was discovered by Sir John Herschel at the Cape of Good Hope with an 18-inch f/13 speculum telescope. He recorded it as "A perfect planetary disc 6 arcsec diameter; quite sharp, with not the least haziness. It is of a most decided independent blue colour when in the field by itself, and with no lamp light and no bright star. About 10' north of it is an orange coloured star 8th mag. When this is brought into view the blue colour of the planetary becomes intense. Shown to my attendant, John Stone, who, on being asked what colour, said at once 'blue.' " His next observation was recorded as "planetary nebula - in light to a star 7th mag; diam. in RA = 1.3 seconds; viewed with all the powers; very beautiful; decidedly blue." On the next occasion he described it as a "planetary nebula, colour a beautiful rich blue, between prussian blue and verditter green. The light is fully = that of a star 8th mag diameter; 2 seconds in RA; 12 arcsec by careful estimation. When kept steadily at rest its outline is sharp and clean, and perhaps a very little elliptic. A feeble lamp light gives it a deep indigo contrasted colour. Ditto if a red star N.p., about 10' distant, be brought into the field with it. My attendant saw it and declared proprio motu that the light has quite a green cast in it. About 90 stars are in the field, none above 11..12 mag, and only one of that magnitude (meaning when the neb. is central). It has none but stars 16th mag near it." Then, on 26 February 1835, after completing the sweep for the night, he viewed it with Maclear: "Blue colour very conspicuous. Has one small companion certain (pos by diagram about 290 ) dist = full diameter, another nearly certain (at about half the distance by diagram, and pos about 135 ) The field is full of stars. Total light of planetary = star of 6th magnitude or 6' m. A very little oval in position about 160 or 165." Some while later, he recorded it as "planetary, diameter 8..10 arcsec, perfectly round and well defined, and of a fine blue colour." His final observation was recorded as "Planetary nebula. Perfectly round, very planetary; colour fine blue; a very little ill defined at the edges; has no 'satellite stars'; very like Uranus, only about half as large again and blue. Diameter in RA = 1.5 seconds."

Hartung writes "it is so bright that even a 2-inch will show the small disk ... this is round, well-defined, vivid pale blue about 10 arcsec across and lies in a fine starry field."

Houston, observing with a 6-inch RTF, writes: "NGC 3918 was recognizable as an 8.5 mag planetary nebula, once its tiny 13 arcsecond disk was ferreted out."

Gerd Bahr-Vollrath (Noosa Heads, Queensland, Australia) observing with an 8-inch f/12 SCT, writes in the The Webb Society Nebulae and Clusters Section Report No. 10, July 1992: "Quite bright and large irregular disc with fainter envelope; appears 'spikey'."

ASV Journal Vol 24 No 3 June 1971: "visible in 1-inch 8x finder."

6-inch f/8.6 Newtonian: A colourless, perfectly round and smooth disk-shaped planetary. In the field with an 8th mag star north-northwest. The nebula, just fainter than 8th mag, is easy to identify; simply rack the eyepiece out of focus, and then start focusing it. As focus is approached, the disk-shaped images of both objects shrink in size. But at an obvious moment, the star continues to shrink, but the planetary remains disk-shaped. The disk is clear at 72x, and possibly even at 40x. (exurban skies) [AS]

10-inch f/5 Newtonian: This is a very interesting object; a 10-inch f/5 at 120x shows it as a small, neat planetary nebula, very bright with a smooth disk and sharply terminated edges. It reminded me of a luminous coin. There is a reddish 8th mag star closeby to its north, and when viewing both in the same field, it is not impossible to imagine the nebula as having a bluish cast. Definitely a good object to study at higher powers. (suburban skies) [AS]

NGC 3960
Bennett 48
Mel 108, Cr 250, Rb 93
RA 11:50:54
Dec -55° 40.0'
Open cluster

Dunlop 349: "a pretty large, faint nebula, 6' or 7' diameter, easily resolvable with slight compression of the stars to the centre, or rather towards the following side of the centre."

h: "cluster, VI class, pretty rich, irregular figure, round with long appendages, gradually pretty much brighter to the middle, 9', stars 13th magnitude."

Trumpler (Lick Obs Bul, Vol 14, No. 420) gives the diameter as 7' and the class as 1 2 m. He notes: "RA of NGC corrected by -3.6 minutes, it must be the same cluster as Melotte 108."

Described in Union Obs. Circulars, 45-76, p 50. "Nebulae, clusters, etc. on Sydney Plates" as "(Dunlop 349)? RA 11h 44.5m Dec -54° 58' (1875) Cluster of 100 stars, 12-14mag., within a radius of 5'."

11x80: Exurban skies, Full Moon: Not found. Suburban skies, dark moon, conditions good, almost near zenith: Nothing found. Surban skies, dark moon, inferior conditions - dew. Picked up this cluster as an extremely faint round glow, 13' across max, with a triangle of stars. Although it is an extremely faint presence, I am confident of the sighting. A challenging object. [AS]

6-inch f/8.6 Newtonian: A gentle round 5 arcmin glow of tiny starpoints, the whole surface being on the verge of resolution. No concentration, stars evenly distributed and all the same brightness. Extremely rich, with no dark areas, central star or dominant members. (exurban skies) [AS]

8-inch Meade Newtonian, 18mm super wide-angle eyepiece: Pretty large open cluster, gradually brighter to the middle. Looks like stars form little arms in a spiral structure to a loose core. One of this extended structures seems a little brighter. Rich open cluster with small pinpoint bright stars in a busy starfield. (exurban skies) [MS]

Stock 15

RA 12:06:54
Dec -59° 28.0'
Open cluster

6-inch f/8.6 Newtonian: Maybe a slightly more dense star field of the milky way, but that's all, folks. Look just over half-degree south-west for a small, perfectly regular parallelogram of four equal 11th mag stars, oriented with long axis pointing almost due north-south. (exurban skies) [AS]

NGC 4230
Cr 253
RA 12:17:12
Dec -55° 06.0'
Open cluster

h: "Cluster class VI. F; pL; irregular; 6'; resolved into stars 13, 14, 15th mag. Place of a star 12th mag, chief and near middle of cluster."

11x80: Binoculars show nothing more definite than a dim star here. [AS]

6-inch f/8.6 Newtonian: This cluster lies due west of F Centaurii, near the Crux border. The cluster is attached to a 9.5m star which forms the right-angle of an isoceles 90-degree triangle; one side (12 arcmin long) points north-south, the other side lies east-west. The 30mm shows perhaps a round, 4 arcmin fuzz, with a 95mag star on its north-west edge. It appears obscure, if at all. With the K9mm eyepiece, 144x, it does not look like a cluster, there being about seven small similarly bright stars, scattered generally eastwards of the 95m one. (exurban skies) [AS]

NGC 4337
Cr 254
RA 12:23:53
Dec -58° 06.0'
Open cluster

h: "A p rich cluster, not m comp M; stars 12..14th mag, in curved branches. A fine double star follows."

Described in Union Obs. Circulars, 45-76, p 50. “Nebulae, clusters, etc. on Sydney Plates” as “Cluster of about 50 stars, 14-16 mag., diameter 3’, with outlying branches, in a rich region.”

6-inch f/8.6 Newtonian: A small cluster between Delta and Gamma Crucis. 30mm shows a fine, delicate grouping, 4 arcmin across, west of an 8th mag double star. There are four stars (3 in a line), much brighter than the rest, congregating on the northern edge of the cluster. The rest of this extremely rich cluster is an irregular mottled glow to the south. With the sweeping power, it is noticed as nebulous and distinct from the background. There is no obvious concentration of stars, the members being evenly distributed. No dark patches apparent. The members show an extreme brightness range, with the majority coming in as mottled. Using K18mm 72x shows about 6 more stars. The double star to the east of the cluster is bright (8th mag) and is cleanly separated at 72x, which shows the southern member as being slightly brighter. (exurban skies) [AS]

Harvard 5
ESO131-SC005, Cr 258, Cr 257
RA 12:27:09
Dec -60° 45.8'
Open cluster

6-inch f/8.6 Newtonian: Cluster south-east of Epsilon Crucis. Least impressive cluster of the evening. With K12.5mm at 104x it is just two stars arranged almost north-south. A much finer view is to be had just 10 arcmin due west, where there is a neat clump of 20 large and small stars in an area 6 arcmin across. (exurban skies) [AS]

NGC 4439
Cr 259, Ld 623, OCL 884.1
RA 12:28:22
Dec -60° 04.0'
Open cluster

Dunlop 300: Using a 9-inch f/12 telescope, Dunlop recorded this cluster on four occassions, describing it as "a triangular group of very small stars, about 3' long, resembling faint nebulae. A star of the 9th magnitude near the north following extremity."

h: "Cluster taken for Dunlop 300; a semi-elliptic group of stars 11..12th mag, diameter 2'."

ASV Journal Vol 24 No 3 June 1971: "small soup ladle-shaped cluster."

10x50: "very dim, no members resolved, right next to a bright star." (exurban skies, dew, no moon) [RH]

11x80: Suburban skies, darkmoon: a small, round after-image of the 8th mag star due north. The orange Epsilon Crucis lies to the southeast. Suburban skies, Full Moon: Reasonably sure I spotted this one, appears as an extended glow to the south-east of an 8th mag star. The Uranometrias show the cluster almost touching the star; I see it further away. Pristine skies: Readily seen as a small, reasonably bright, round globular cluster, with an 8th magnitude star just north-west. [AS]

6-inch f/8.6 Newtonian: Cluster inside Crux, east-northeast of Epsilon. The sweeping power shows it as an obvious cluster, about 4 arcmin across. An evident half-circle shape, and with some stars in the centre, making an epsilon, or "element of" symbol. There is a bright star (with a small companion) close to the north-west (by rough sketch I made, this is at least 4 arcmin distant) [Note Dunlop's error, placing the star to the north-east]. The cluster displays a moderate brightness range, is well detached, and shows no clear concentration. With K9mm at 144x, 11 stars are seen to make up the curve, with two on the central bar. With the aperture stop (50mm) in place, the cluster is lost, and a nebulous round patch, with a brighter patch in the north, is seen. (exurban skies) [AS]

Ru 165
ESO172-SC001
RA 12:28:33
Dec -56° 26.3'
Open cluster

The SAC 4.0 database comments: "Asterism?"

10x50: "two star members seen, background fuzz of unresolved stars, rather faint appearance and very small." [RH]

11x80: Does not impress me as an open cluster: only 2 bright stars and 5 fainter stars can be seen. Suburban skies: Using averted vision, looks like a fuzzy patch or unresolved stars. Exurban skies, Full Moon: With 9.5 mag stars difficult, this cluster doesn't show more than 4 tiny stars scattered around a bright roughly central luminary. There is another bright star, roughly between the cluster and nearby Gamma Cru. This star appears reddish. Pristine skies: Very poor, coarse cluster of stars; maximum ten members, thus hardly a spectacular grouping. Two almost equally bright stars within, both appearing reddish, especially the eastern-most one. [AS]

6-inch f/8.6 Newtonian: A coarse cluster north and west of gamma Crucis. 30mm eyepiece shows it as not much of a cluster, and very coarse. As such, it is not detached from the background, and has a lob-sided M shape. Great brightness range: one bright star, near the centre, which has a slight orange colour, then half-dozen fainter members, with maybe another 6 extremely faint, scattered around. In comparison, a similar-sized field to the north-east has almost as many stars. There is also a bright, 6th mag orange star on the eastern edge; it does not look like a cluster member in the 30mm field of view, as it is just too far away. (suburban skies) [AS]

15.5-inch f/9 Newtonian: This interesting open cluster, as seen through a 15.5-inch reflector, has a very bright orange stars on its southern side, with a slightly less bright but equally orange star opposite. There are a further 3 stars fainter than these two, and then about half dozen stars pretty much fainter. It is quite large, spanning about 17' across, making it a very loose scattering of stars. (suburban skies) [AS]

Hogg 14
ESO131-SC007
RA 12:28:35
Dec -59° 49.1'
Open cluster

The SAC 4.0 database comments: "Asterism?"

6-inch f/8.6 Newtonian: A small cluster in Crux, roughly north of another small cluster, NGC 4439. The sweeper eyepiece shows a small nebulous glow. With K18mm at 72x, the cluster shows as an irregularly round fuzzy patch, with a 10th mag star on the western edge, and maybe three more very small stars. Stands out from the surrounding field. Tried other eyepieces; higher power doesn't help - more aperture is needed to make it out satisfactorily. (exurban skies) [AS]

15.5-inch f/9 Newtonian: This pleasing cluster consists of an angular arc of 6 prominent stars with a central line of two, with a total of about a dozen stars, the others being considerably faint. The central bar lies west-east, and forms an arrow pointing to the east. The first pattern the eye traces here is of the arc, but then it sees the arrow-asterism. The cluster measures 4' north-south and about 2.5 west-east. It is easy to spot since it has a regular shape and stands out well from the background starfield. North and slightly west of the cluster in the same half degree field is an 8th mag star with a fainter companion further north. (suburban skies) [AS]

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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 March 01