U 362
07:40 to 08:20
-28° to -39°
Pup
Jan-Apr

FEATURED OBJECTS: Boch 15, Haff 13, NGC 2439, Ru 30, Ru 31, ESO368-SC011, Haff 14, NGC 2451, Haff 15, Ru 35, ESO368-SC014, Cz 32, Haff 17, NGC 2477, Sanduleak 2-18, Ru 152, NGC 2489 (Ben 38), Haff 20, Ru 44, Ru 43, Ru 153, Ru 47, NGC 2520, Ru 48, Ru 50, Ru 51, ESO430-SC014, ESO369-PN004, Ru 155, Ru 52, NGC 2527, ESO430-SC018, NGC 2533, vdBH 19, ESO369-PN005, Ru 54, NGC 2546, Ru 55, vdBH 23, Ru 58, Haff 26, NGC 2568, NGC 2567, NGC 2571, Ru 59.

Boch 15

RA 07:40:04
Dec -33°32.0'
Open cluster

Steve Coe, observing with a 13” f/5.6, notes: “Faint, pretty small, not rich, compressed at 165X. There are six stars in this cluster, including a 9th mag star on the east side. The cluster has a fuzzy backround. High power helps this compact cluster, it was barely noticed at 100X.”

10-inch f/5 Newtonian: At 30x this cluster appears very obscure; it shows as a 9th mag star, and close to its west, a nebulous feature. This nebulous patch can just be resolved into stars at 66x, while 120x shows it clearly as four faint stars. (suburban skies) [AS]

Haff 13
ESO429-SC010
RA 07:40:28
Dec -30°04.7'
Open cluster

10-inch f/5 Newtonian: In a 10-inch it looks like a smaller version of a typical Collinder cluster, four reasonably bright members with about 15 smaller stars making up a non-descript open cluster. The stars form a triangle with the sharp point pointing south-west. Opposite the northeastern base of the triangle is a dim line of three faint stars, more clearly seen at 66x. On the inside of the triangle lie two 9th mag stars and together with four other small stars form an elongated V. Besides these stars, about 5 more are visible within the confines of the triangle. The 30x eyepiece actually shows it as an open cluster (as opposed to merely an asterism). (suburban skies) [AS]

NGC 2439
Mel 74, Cr 158, Rb 61
RA 07:40:46
Dec -31°38.0'
Open cluster

Discovered by Sir John Herschel at the Cape of Good Hope with an 18-inch f/13 speculum telescope. He recorded it as "a cluster of about 150 stars, B, pL, p rich, not much more compressed to the middle, 8' diameter, has one star 8th mag, one red one 9th mag, the rest 12..14th mag."

Trumpler (Lick Obs Bul, Vol 14, No. 420) gives the diameter as 9' and the class as 2 3 mU.

Tom Lorenzin, in the electronic version of "1000+ The Amateur Astronomers' Field Guide to Deep Sky Observing", notes: “7.5M; 9' diameter; rich and compact; 50-plus 9M and dimmer members; contains the 6.5M VAR ST R PUP as its brightest member.”

Steve Coe, observing with a 13” f/5.6, notes: “Bright, large, pretty rich, 42 stars counted at 100X. The center of this cluster is dark and this bizarre absorption from dark nebulae makes the cluster take on a horseshoe or "Arc de Triumph" shape.”

10-inch f/5 Newtonian: This little cluster, like NGC 2362 around Tau CMa, nicely demonstrates the efficacy of averted vision in a 10-inch f/5 at 30x. On the northeastern edge of the cluster is a red star known as R Puppis. Looking directly at this star, you see to its south and west six or so smaller stars, irregularly distributed. But averted vision on any of the stars in this rich milky way field, especially a fine, close double star lying nearby, shows a sheen of stars filling up the space to the southwest of the red variable. A 66x eyepiece, with increased contrast, clearly shows these cluster members, as well as a very nice close double to the west and south of R Puppis. There appear to be quite a number of paired groupings in the cluster, which overall seems box /shaped. The number of stars easily seen are 8, but it is clear that there are many fainter stars providing a background glow for this interesting object. At 66x the brighter cluster members are easily visible, so averted vision doesn't function as breathtakingly as when a low-power eyepiece is used. (suburban skies) [AS]

Ru 30
ESO429-SC015
RA 07:42:23
Dec -31°28.4'
Open cluster

10-inch f/5 Newtonian: A 10-inch f/5 at 30x shows this cluster as a more or less triangular patch of light, reasonably small and nebulous. At 66x it appears as an equilateral triangle of very similar-magnitude, reasonably faint stars. (suburban skies) [AS]

Ru 31
ESO368-SC009
RA 07:42:57
Dec -35°35.7'
Open cluster

10-inch f/5 Newtonian: This cluster is quite noticeable in a 10-inch f/5 at 30x as a nebulous patch surrounding a 9th mag star. At 120x it appears as a small gathering of about 6 stars (one of which is 9th mag) lying in a sharp triangular grouping pointing south. These are the only members visible. The cluster is flanked on its east and west by two 9th mag stars. (suburban skies) [AS]

ESO368-SC011

RA 07:44:22
Dec -34°38.7'
Open cluster

Haff 14
ESO429-SC016
RA 07:44:51
Dec -28°22.4'
Open cluster

NGC 2451
Cr 161
RA 07:45:24
Dec -37°57.0'
Open cluster

h: "The chief star (4th mag) of an orange colour, of a very large and very diffused cluster of large stars, too loose to be a fit object for the ordinary magnifying power."

Trumpler (Lick Obs Bul, Vol 14, No. 420) gives the diameter as 37' and the class as 1 3 p.

See: Williams P M "Photometry of NGC 2451" MNASSA p122 10.15.2 ["Three colour photoelectric observations have been made of 82 stars in and near the open cluster NGC 2451 using the 24-inch Victoria Refractor and the 40-inch Elizabeth Reflector at the Cape. From the colour-mag diagram, as well as from CPC proper motions, it was seen that the grouping of stars hitherto believed to comprise the whole cluster is but the nucleus of a larger cluster about three times as large. The diameter of this cluster is about 2° or 12 parsecs." A diagram of the cluster nucleus is included]; Williams P M "Photoelectric photometry of NGC 2451" MNASSA p30 10.15.2 ["Three-colour photometric resulys are presented for 213 stars in the region of the open cluster NGC 2451" A detailed diagram of stars in the nucleus is also included]; Williams P M "The Open Cluster NGC 2451" MNASSA p139 10.15.2 ["From photometric data previously given the distance of NGC 2451 is found to be 330±20 pc and the age about 23 million years. It is suggested, from a comparison of data, including space motions of this cluster and Collinder 140 that they, perhaps together with Collinder 135 and Collinder 173, are the remaining nuclei of an early-type association which has broken up"].

Harrington notes that "thirty [of the stars in the cluster] are resolvable in 11-power binoculars. The group's brightest star, orange-red c Puppis, stands out among the crowd of white and blue-white suns. Collectively, the cluster forms a colorful welcome mat to the southern sky." He adds that it is best viewed "through either binoculars or a wide-field telescope, as the cluster spans 45 arc minutes."

Tom Lorenzin, in the electronic version of "1000+ The Amateur Astronomers' Field Guide to Deep Sky Observing", notes: “2.8M; 45' diameter; very, very bright and large! 40-plus 6 thru 8M members plus 3.5M c PUP (SAO 198398); cluster N2477 is 1.5 degrees to ESE; great binocular object!.”

Glen Cozens notes that "even binoculars show its spray of starlight well, appearing as a scorpion seen face on with its tail raised high. A bright orange star marks its head."

Steve Coe, observing with a 13” f/5.6, notes: “Bright, very, very large, scattered. 36 stars counted at 60X, with one yellow 4th mag and 35 others mags 7 to 11. 10 stars are resolved in the 11 X 80 finder.”

Todd Gross, in a submission to the IAAC, reports an observation with an 80mm APO refractor: “This is a very nice cluster at low power. It is a fairly large loose cluster that spirals out in arms with about 2 dozen stars from a red star near it's center. Stars are fairly uniform in brightness, with the red star the brightest. Did not even try to go higher as it would have lost it's "cluster" look with more magnification.”

11x80: Viewing with 11x80 binoculars, this cluster contrasts nicely with the nearby NGC 2477, both very easy to find. The two clusters are totally different in appearance. NGC 2451 is a very large, coarse, scattered cluster, with a bright orange primary. Even under poorer conditions, is shows as a splendid and extremely coarse and bold cluster with a bright red primary near the centre. (suburban skies) [AS]

10-inch f/5 Newtonian: In a 10-inch f/5 at 30x this cluster looks like a rich Collinder-type object. Near the centre of the cluster is the prominent orange c Puppis. The cluster fits very nicely into a one degree field, having about 15 brighter memebrs and may more smaller stars. An attractive if somewhat spread-out group. The brighter members are clearly visible in the finder. (suburban skies) [AS]

Haff 15
ESO368-SC012
RA 07:45:31
Dec -32°50.5'
Open cluster

Steve Coe, observing with a 13” f/5.6, notes: “Pretty bright, pretty small, very compressed, not rich at 165X. Faint fuzzy backround of unresolved stars at all powers.”

10-inch f/5 Newtonian: A 10-inch f/5 at 30x shows this as a mottled nebulous patch in a very busy milky way starfield. The cluster's southern edge is marked by three stars lying in an east-west curve. These are the brightest stars in this obscure grouping. A further three small stars to the north give it a general triangular appearance. The most remarkable feature is the curve of three bright stars; the fainter haze extending to the north from this baseline makes one think of a plate of steaming soup!(suburban skies) [AS]

Ru 35
ESO429-SC018
RA 07:46:12
Dec -31°17.0'
Open cluster

ESO368-SC014

RA 07:47:03
Dec -32°58.2'
Open cluster

Cz 32
King 24, ESO429-SC020
RA 07:50:28
Dec -29°51.1'
Open cluster

Haff 17
ESO429-SC022
RA 07:51:36
Dec -31°48.8'
Open cluster

NGC 2477
Mel 78, Cr 165, Rb 65
RA 07:52:17
Dec -38°32.0'
Open cluster

This open cluster was discovered by Lacaille and included in his 1755 catalogue as Class I No. 3, classifying it as a nebula. In his half-an-inch 8x telescope he saw it as a "big nebula 15' to 20' diameter."

James Dunlop observed this object from Paramatta, New South Wales, and included it as No. 535 in his catalogue of 1827. Using a 9-inch f/12 telescope, he described it as "a pretty large faint nebula, easily resolvable into small stars, or rather a cluster of very small stars, with a small faint nebula near the north preceding side, which is rather difficult to resolve into exceedingly small stars. This is probably two clusters or nebula in the same line; the small nebula is probably three times the distance of the large nebula." Dunlop recorded this cluster on 5 occassions.

h: "Superb cluster, gbM, 20' diameter, much more than fills the whole field. Stars 10 and 11th mag all nearly equal." On a second occassion he called it "Cluster 6th class, bright, large, rich, not very highly condensed in the middle. Stars very remarkably equal. All 12 or 13th mag. Very few 14th mag; none 11th mag. A fine object." His third observation was recorded as "a very beautiful large cluster, very rich; stars nearly equal, and 12th mag, gbm, not much compressed in the middle; more than fills the field. (N.B. It is visible in the finder of the equatorial, and in the telescope of that instrument appears as a fine cluster."

Burnham calls this "probably the finest of the galactic clusters in Puppis." The NGC calls it a remarkable cluster, rich and well spread-out, consisting of stars of 12th magnitude. Burnham notes that it is a "striking group, somewhat smaller than M46, but richer and more compact." P. Doig called it "almost globular" and Shapely wrote of it as "in superficial appearance... the richest of galactic clusters; or perhaps it is the loosest of globular clusters."

Hartung writes that the cluster is "broadly concentrated to a dense centre of 12'; the stars are very numerous and many are grouped in curved lines and sprays with dark sky between, making a beautiful effect. A 6" shows this cluster fairly well."

Harrington says the cluster "appears like a ball of celestial cotton spanning about a Moon's diameter when viewed through low-power binoculars. With a rich-field telescope, the cluster's fuzziness dissolves into a myriad of faint points of light. In all, 160 stars dwell within NGC 2477, though none shine brighter than 10th magnitude."

Glen Cozens notes that "a moderate aperture will show it as well-resolved stars against a grainy background of faint starlight."

Tom Lorenzin, in the electronic version of "1000+ The Amateur Astronomers' Field Guide to Deep Sky Observing", notes: “6M; 25' diameter; hundreds of 10M and dimmer members; use wide field at 50x; great binocular object just N of 4M b PUP.”

Steve Coe, observing with a 13” f/5.6, notes: “Bright, large, very, very rich, very compressed. 180 total members estimated by counting 45 stars in the northeast quadrant at 100X. There are many lovely dark lanes that wind there way through several star chains and an ever-present glowing backround of more stars. I can resolve 20 stars in the 11X80 finder.”

11x80: A really beautiful sight; 11x80 binoculars show it as a large round, nebulous patch, with no stars; a bright star, b Pup, lies to its southeast. The cluster is easy to locate, since it lies north of the pretty bright b Puppis. A hasty glance shows nothing, but the slightest averted vision shows a glorious glow, a faint glimmer of starlight, which is remarkabley large. This is quite unexpected, because you don't expect a patch of barren sky to suddenly burst into a puff of starlight. It looks like the faint extended halo of a comet. Contrasts nicely with nearby NGC 2451. Even poor conditions, with light pollution and haze, don’t spoil it; it remains a fantastic sight, appearing as a perfectly insubstantial object. It is difficult to judge its shape - I would suggest it appears round. This cluster is the slightest of glows imaginable, not a star in sight - remarkable! (suburban skies) [AS]

6-inch f/8.6 Newtonian: What a splendid object! Exquisitely minute stars almost fill the half-degree field of view. The cluster appears distinct from the background sky, a myriad stars evenly but densely spread out. This extremely rich gathering has no central star or otherwise dominant member. There is a chain of stars leading off to the north-east. The dark lanes are very noticeable in this cluster. The cluster has a bright triangular stellar region, defined on the east and north by the two dark lanes, which intersect at an almost 90 degree angle. The eastern dark lane ends in a definite bulbous lobe, which is the most prominent in the cluster. The dark lane making the southern edge also has a bulbous ending; the cluster seems to vaguely extend beyond this barrier. These two dark lanes look somewhat like golfclubs, crossed near their handles with the heads facing inwards. The effect of the dark lanes on the shape of the cluster is quite noticeable. At low (finding) power initially, and afterwards, the impression is created that the cluster is box-shaped, with the eastern edge more sharply outlines. (exurban skies) [AS]

10-inch f/5 Newtonian: A 10-inch f/5 at 30x evenly resolves the cluster into small stars; it appears just under a third of a degree across, and although it has an irregular outline, the stars are pretty evenly distributed across the surface; there does, however, appear to be a more concentrated triangular region cutting right across the cluster's surface. At 66x, about half a dozen brighter-than-average (10th mag) stars are distributed across the clusters surface, causing it to appear lumpy and irregularly condensed. The textured appearance of this remarkable cluster is most pleasing. It really is a most beautiful sight, and forms a nice contrast with the bright star (b Pup) which can be seen in the same field; it sort of looks as if once there were two bright stars here, and one suddenly disintegrated into faint shards of light. (suburban skies) [AS]

Sanduleak 2-18
ESO369-PN002
RA 07:52:55
Dec -36°43.8'
Planetary nebula

Ru 152
ESO311-SC019
RA 07:54:28
Dec -38°14.1'
Open cluster

NGC 2489
Bennett 38, Mel 79, Cr 169, Rb 66
RA 07:56:12
Dec -30°03.0'
Open cluster

Discovered in 1785 by William Herschel (H VII-023) with an 18.7-inch f/13 speculum telescope. He called it "a compressed cluster of pretty large stars, considerably rich."

James Dunlop observed this object from Paramatta, New South Wales, and included it as No. 626 in his catalogue of 1827. Using a 9-inch f/12 telescope, he described it as "a cluster of small stars, of an irregular round figure, with faint nebula, easily resolvable. The 257 Argus is south following."

h: "Cluster 7th class. Round, 5' diameter, stars 12th mag." On a second occassion he called it "A round, pretty compressed cluster of stars 11..13th mag; 6th or 7th class; gradually brighter in the middle, pretty rich, 7' diameter."

Listed by the Herschel Club, described as “some 30 stars, small, faint stars, stands out well, circular in shape, two bright stars stand out within cluster. 8-inch, 48x.”

Tom Lorenzin, in the electronic version of "1000+ The Amateur Astronomers' Field Guide to Deep Sky Observing", notes: “7.9M; 8' diameter; small and scattered; 35-plus 11M and dimmer members; bright star to SE is 5M SAO 198636.”

Steve Coe, observing with a 13” f/5.6, notes: “Bright, pretty large, pretty rich, not compressed, 31 stars in nice chains counted at 100X. Seen in 11X80 finder.”

Haff 20
ESO430-SC004
RA 07:56:13
Dec -30°22.2'
Open cluster

Steve Coe, observing with a 13” f/5.6, notes: “Faint, pretty small, compressed, 6 stars of mags 12 and dimmer, with a hazy backround at 135X.”

Ru 44
ESO430-SC005
RA 07:58:51
Dec -28°35.0'
Open cluster

Ru 43
ESO430-SC006
RA 07:59:17
Dec -28°58.2'
Open cluster

Ru 153
ESO430-SC007
RA 08:00:18
Dec -30°17.0'
Open cluster

Ru 47
ESO430-SC008
RA 08:02:19
Dec -31°04.4'
Open cluster

NGC 2520

RA 08:02:30
Dec -28°11.0'
Open cluster

Observed by Sir John Herschel at the Cape of Good Hope with an 18-inch f/13 speculum telescope. He recorded it as "Cluster 7th class, distinguished among milky way clusters, pretty rich, bright. The star taken is the chief of a condensed hook in the following part." In "Results of Astronomical Observations .. at the Cape of Good Hope" (1847), Herschel notes that this object is number 488 in his Slough Catalogue and VIII 30 in his father's catalogue. Dreyer's NGC assigns the NGC number 2527 to these two entries.

The RNGC (Sulentic and Tifft 1973) notes that this is a nonexistent object. Their coded description reads NOCL S.

Ru 48
ESO430-SC011
RA 08:02:41
Dec -32°02.4'
Open cluster

Ru 50
ESO430-SC012
RA 08:03:26
Dec -30°51.6'
Open cluster

Ru 51
ESO430-SC013
RA 08:03:36
Dec -30°38.5'
Open cluster

ESO430-SC014

RA 08:03:37
Dec -31°25.6'
Open cluster

ESO369-PN004
PK251-01.01
RA 08:04:12
Dec -34°16.0'
Planetary nebula

Ru 155
ESO430-SC016
RA 08:05:04
Dec -31°48.6'
Open cluster

Ru 52
ESO430-SC017
RA 08:05:08
Dec -31°58.3'
Open cluster

NGC 2527
Cr 174
RA 08:05:17
Dec -28°08.0'
Open cluster

Discovered in 1785 by William Herschel (H VIII-030) with an 18.7-inch f/13 speculum telescope. He called it "a very large cluser of many coarsely scattered large stars."

Listed by the Herschel Club, described as “some 50 stars, loose and scattered cluster, somewhat shapeless, stars of similar magnitude. 8-inch, 48x.”

Tom Lorenzin, in the electronic version of "1000+ The Amateur Astronomers' Field Guide to Deep Sky Observing", notes: “7M; 20' diameter; large and medium rich; 40-plus 11M and dimmer members.”

Steve Coe, observing with a 13” f/5.6, notes: “Bright, very large, pretty rich, somewhat compressed, 36 stars of mags 9 to 13 fill the field with nice chains at 100X.”

6-inch f/8.6 Newtonian: Large, faint cluster, its small stars spread out over a large rich field. Most of the stars are of the same, small, magnitude. In the sweeper eyepiece (42x, 50 arcmin), the cluster appears as a slightly elongated triangle, pointing north-east, where the brightest star also lies, forming the tip. The north-south side of this triangle measures 12 arcmin. The cluster is quite lost in this wide field, and is not well separated from the rich background. A higher power of 72x on a half-degree field shows the cluster better, but the field is still immensely rich and the cluster perhaps too spread out. (exurban skies, lim mag 6.0 (naked eye), seeing very good.) [AS]

ESO430-SC018

RA 08:06:52
Dec -30°50.2'
Open cluster

NGC 2533
Cr 175
RA 08:07:00
Dec -29°52.0'
Open cluster

h: "pretty compressed cluster sixth class, irregularly round, stars 13..14th mag. One = about 8th mag near the middle."

Tom Lorenzin, in the electronic version of "1000+ The Amateur Astronomers' Field Guide to Deep Sky Observing", notes: “8M; 5' diameter; fairly small and medium rich; 40-plus 12M and dimmer members.”

Steve Coe, observing with a 13” f/5.6, notes: “Pretty bright, pretty large, compressed at 135X. There is one star of 9th mag and 15 more of mags 12 to 13, then a fuzzy backround of unresolved stars.”

vdBH 19
ESO430-SC021
RA 08:07:04
Dec -32°21.4'
Open cluster

ESO369-PN005
PK250+00.01
RA 08:08:57
Dec -32°15.8'
Planetary nebula

Ru 54
ESO430-SC023
RA 08:11:20
Dec -31°56.8'
Open cluster

NGC 2546
Cr 178
RA 08:12:23
Dec -37°37.0'
Open cluster

This cluster was discovered by Lacaille and included in his 1755 catalogue as Class II No. 4. With the naked eye, he called it "two confused groups"; in his half-an-inch 8x telescope he saw it as "many close faint stars."

James Dunlop observed this object twice from Paramatta, New South Wales, and included it as No. 563 in his catalogue of 1827. Using a 9-inch f/12 telescope, he described it as "a large cluster of stars of mixt magnitude, rather extended figure, not rich in very small stars."

h: "a cluster 8th class of about 20 bright stars in an oblong, 8' long, 3' broad." On a second occassion he called it "chief triangle of stars 9, 10, 11th mag of an oblong irregular cluster." His third observation was recorded as "a bright group in full part of a bright, not rich, irregular oblong cluster, 6' long, 3 or 4' broad."

Trumpler (Lick Obs Bul, Vol 14, No. 420) gives the diameter as 45' and the class as 3 2 p.

Harrington writes that "rich-field telescopes reveal an isosceles triangle of 7th- and 8th-magnitude stars framing about 20 stars of 9th magnitude and fainter."

Tom Lorenzin, in the electronic version of "1000+ The Amateur Astronomers' Field Guide to Deep Sky Observing", notes: “7M; 25' diameter; large, round and sparse; 50-plus 9M and dimmer members; binocular object.”

Steve Coe, observing with a 13” f/5.6, notes: “Very bright, very large, scattered, not rich, not compressed. 62 stars counted at 60X, one is a lovely dark yellow star on the south side of the cluster. This large cluster is easy in the 11X80 finder.”

11x80: In binoculars the cluster looks like a brighter patch of the Milky Way. An 11x80 shows a large area, about a degree, sprinkled with very many faint small stars, but not too faint to be resolved. It shows as a faint and rich starfield making an irregular form defying classification. About a degree away lie a pair of double stars, one bright and close, the other pair slightly fainter and more distant. (suburban skies) [AS]

10-inch f/5 Newtonian: This is a very striking open cluster when viewed with a 10-inch f/5 at 30x. It appears quite suddenly out of the rich milky way background as an approx. one degree patch of even-brighter milky way background. The cluster seems to lie in a rectangular grouping, elongated roughly north-south. It is very large, and the stars are irregularly scattered across a wide field, forming a loose swathe of stars. On the western edge, just to the south of a pretty bright star, is a tight, elongated knot of stars. Looking at the cluster in the field of view, it looks just like a bright milky way starfield, but when you move the 'scope a bit off and compare it with the real background starfield, it is seen as being something more than just a busy field. (suburban skies) [AS]

Ru 55
ESO430-SC025
RA 08:12:25
Dec -32°35.0'
Open cluster

The SAC 4.0 database comments: "Asterism?"

vdBH 23

RA 08:14:23
Dec -36°23.0'
Open cluster

Ru 58
ESO430-SC027
RA 08:14:47
Dec -31°56.9'
Open cluster

Haff 26
ESO430-SC029
RA 08:15:38
Dec -30°49.8'
Open cluster

NGC 2568
Pismis 1
RA 08:17:42
Dec -37°05.0'
Open cluster

Oddly missed by the Herschels, it was picked up by E E Barnard, who called it “vF, pL, F * inv”.

Steve Coe, observing with a 13” f/5.6, notes: “Faint, pretty small, not rich, somewhat compressed, 6 stars at 150X, 2 about 11th mag and 4 of 13th mag.”

10-inch f/5 Newtonian: In a 10-inch f/5 at 30x this cluster appears as a faint nebulous patch in a bright milky way field. With averted vision, maybe two stars are glimpsed. (suburban skies) [AS]

NGC 2567
Mel 86, Cr 180, Rb 73
RA 08:18:36
Dec -30°38.0'
Open cluster

Discovered in 1793 by William Herschel (H VII-064) with an 18.7-inch f/13 speculum telescope. He called it "a large cluster of stars of a middling size. iE, considerably rich. The stars are chiefly in rows."

h: "middle of cluster, not very rich, irregularly round, not much compressed, 10' diameter. Stars 12..15th mag, few very minute." On a second occassion he called it "a pretty rich cluster of about 60 stars, 12..13th mag, irregularly round, glbM, 8' diameter."

Trumpler (Lick Obs Bul, Vol 14, No. 420) gives the diameter as 11' and the class as 2 2 m. The RNGC (Sulentic and Tifft 1973) notes that this is a 8.5 mag open cluster.

Listed by the Herschel Club, described as “some 50 stars, situated in fairly rich field. Bright stars mingled with fainter ones, a very pretty cluster, somewhat scattered. 8-inch, 48x.”

Tom Lorenzin, in the electronic version of "1000+ The Amateur Astronomers' Field Guide to Deep Sky Observing", notes: “8M; 10' diameter; fairly rich and compressed; 50-plus 11 thru 14M members; SW-most of a neat group of four clusters.”

Steve Coe, observing with a 13” f/5.6, notes: “Pretty bright, pretty large, pretty rich, 42 stars counted at 135X. There are several nice, curved chains of stars within this cluster.”

NGC 2571
Cr 181
RA 08:18:58
Dec -29°44.0'
Open cluster

Discovered in 1793 by William Herschel (H VI-039) with an 18.7-inch f/13 speculum telescope. He called it "a cluster of large stars considerably rich, iR, above 15' diameter."

Trumpler (Lick Obs Bul, Vol 14, No. 420) gives the diameter as 10' and the class as 1 3 p. The RNGC (Sulentic and Tifft 1973) notes that this is a 7.5 mag open cluster.

Listed by the Herschel Club, described as “25 stars counted in this loose and irregular grouping. Mags of stars similar, somewhat faint. 8-inch, 48x.”

Tom Lorenzin, in the electronic version of "1000+ The Amateur Astronomers' Field Guide to Deep Sky Observing", notes: “7M; 10' diameter; fairly large and sparse; 30-plus 8M and dimmer members.”

Steve Coe, observing with a 13” f/5.6, notes: “Pretty bright, pretty large, pretty rich, somewhat compressed, 30 stars of mags 9 to 13 counted at 135X.”

11x80: As seen with 11x80 binoculars, the cluster shows only 3 or so brighter members surrounded by a faint smudge of dim stars.(suburban skies) [AS]

Ru 59
ESO370-SC007
RA 08:19:21
Dec -34°28.9'
Open cluster

The SAC 4.0 database comments: "Asterism?"

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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